Zobrazeno 1 - 10
of 43
pro vyhledávání: '"Villaseñor, Jesus Noel"'
Autor:
Bozhilov, Vladimir, Antonova, Desislava, Hobson, Melissa J., Brahm, Rafael, Jordan, Andres, Henning, Thomas, Eberhardt, Jan, Rojas, Felipe I., Batygin, Konstantin, Torres-Miranda, Pascal, Stassun, Keivan G., Millholland, Sarah C., Stoeva, Denitza, Minev, Milen, Espinoza, Nestor, Ricker, George R., Latham, David W., Dragomir, Diana, Kunimoto, Michelle, Jenkins, Jon M., Ting, Eric B., Seager, Sara, Winn, Joshua N., Villasenor, Jesus Noel, Bouma, Luke G., Medina, Jennifer, Trifonov, Trifon
Publikováno v:
ApJL 946 L36 (2023)
We report the discovery of a super-Jovian 2:1 mean-motion resonance (MMR) pair around the G-type star TIC 279401253, whose dynamical architecture is a prospective benchmark for planet formation and orbital evolution analysis. The system was discovere
Externí odkaz:
http://arxiv.org/abs/2302.10838
Autor:
Mann, Christopher R., Lafrenière, David, Dragomir, Diana, Quinn, Samuel N., Tan, Thiam-Guan, Collins, Karen A., Howell, Steve B., Ziegler, Carl, Mann, Andrew W., Stassun, Keivan G., Kristiansen, Martti H., Osborn, Hugh, Boyajian, Tabetha, Eisner, Nora, Hellier, Coel, Ricker, George R., Vanderspek, Roland, Latham, David W., Seager, S., Winn, Joshua N., Jenkins, Jon M., Villaseñor, Jesus Noel, McLean, Brian, Rowden, Pamela, Torres, Guillermo, Caldwell, Douglas A., Collins, Kevin I., Schwarz, Richard P.
We present a validation of the long-period ($91.68278^{+0.00032}_{-0.00041}$ days) transiting sub-Neptune planet TOI-1221 b (TIC 349095149.01) around a Sun-like (m$_{\rm V}$=10.5) star. This is one of the few known exoplanets with period >50 days, an
Externí odkaz:
http://arxiv.org/abs/2209.13651
Autor:
Espinoza, Néstor, Pallé, Enric, Kemmer, Jonas, Luque, Rafael, Caballero, José A., Cifuentes, Carlos, Herrero, Enrique, Béjar, Víctor J. Sánchez, Stock, Stephan, Molaverdikhani, Karan, Morello, Giuseppe, Kossakowski, Diana, Schlecker, Martin, Amado, Pedro J., Bluhm, Paz, Cortés-Contreras, Miriam, Henning, Thomas, Kreidberg, Laura, Kürster, Martin, Lafarga, Marina, Lodieu, Nicolas, Morales, Juan Carlos, Oshagh, Mahmoudreza, Passegger, Vera M., Pavlov, Alexey, Quirrenbach, Andreas, Reffert, Sabine, Reiners, Ansgar, Ribas, Ignasi, Rodríguez, Eloy, López, Cristina Rodríguez, Schweitzer, Andreas, Trifonov, Trifon, Chaturvedi, Priyanka, Dreizler, Stefan, Jeffers, Sandra V., Kaminski, Adrian, López-González, María José, Lillo-Box, Jorge, Montes, David, Nowak, Grzegorz, Pedraz, Santos, Vanaverbeke, Siegfried, Osorio, Maria R. Zapatero, Zechmeister, Mathias, Collins, Karen A., Girardin, Eric, Guerra, Pere, Naves, Ramon, Crossfield, Ian J. M., Matthews, Elisabeth C., Howell, Steve B., Ciardi, David R., Gonzales, Erica, Matson, Rachel A., Beichman, Charles A., Schlieder, Joshua E., Barclay, Thomas, Vezie, Michael, Villaseñor, Jesus Noel, Daylan, Tansu, Mireies, Ismael, Dragomir, Diana, Twicken, Joseph D., Jenkins, Jon, Winn, Joshua N., Latham, David, Ricker, George, Seager, Sara
We report the discovery and characterization of TOI-1759~b, a temperate (400 K) sub-Neptune-sized exoplanet orbiting the M~dwarf TOI-1759 (TIC 408636441). TOI-1759 b was observed by TESS to transit on sectors 16, 17 and 24, with only one transit obse
Externí odkaz:
http://arxiv.org/abs/2202.01240
Autor:
Dalba, Paul A., Kane, Stephen R., Dragomir, Diana, Villanueva Jr., Steven, Collins, Karen A., Jacobs, Thomas Lee, Lacourse, Daryll M., Gagliano, Robert, Kristiansen, Martti H., Omohundro, Mark, Schwengeler, Hans M., Terentev, Ivan A., Vanderburg, Andrew, Fulton, Benjamin, Isaacson, Howard, Van Zandt, Judah, Howard, Andrew W., Thorngren, Daniel P., Howell, Steve B., Batalha, Natalie M., Chontos, Ashley, Crossfield, Ian J. M., Dressing, Courtney D., Huber, Daniel, Petigura, Erik A., Robertson, Paul, Roy, Arpita, Weiss, Lauren M., Behmard, Aida, Beard, Corey, Brinkman, Casey L., Giacalone, Steven, Hill, Michelle L., Lubin, Jack, Mayo, Andrew W., Močnik, Teo, Murphy, Joseph M. Akana, Polanski, Alex S., Rice, Malena, Rosenthal, Lee J., Rubenzahl, Ryan A., Scarsdale, Nicholas, Turtelboom, Emma V., Tyler, Dakotah, Benni, Paul, Boyce, Pat, Esposito, Thomas M., Girardin, E., Laloum, Didier, Lewin, Pablo, Mann, Christopher R., Marchis, Franck, Schwarz, Richard P., Srdoc, Gregor, Steuer, Jana, Sivarani, Thirupathi, Unni, Athira, Eisner, Nora L., Fetherolf, Tara, Li, Zhexing, Yao, Xinyu, Pepper, Joshua, Ricker, George R., Vanderspek, Roland, Latham, David W., Seager, S., Winn, Joshua N., Jenkins, Jon M., Burke, Christopher J., Eastman, Jason D., Lund, Michael B., Rodriguez, David R., Rowden, Pamela, Ting, Eric B., Villaseñor, Jesus Noel
We report the discovery of TOI-2180 b, a 2.8 $M_{\rm J}$ giant planet orbiting a slightly evolved G5 host star. This planet transited only once in Cycle 2 of the primary Transiting Exoplanet Survey Satellite (TESS) mission. Citizen scientists identif
Externí odkaz:
http://arxiv.org/abs/2201.04146
Autor:
Wong, Ian, Shporer, Avi, Zhou, George, Kitzmann, Daniel, Komacek, Thaddeus D., Tan, Xianyu, Tronsgaard, René, Buchhave, Lars A., Vissapragada, Shreyas, Greklek-McKeon, Michael, Rodriguez, Joseph E., Ahlers, John P., Quinn, Samuel N., Furlan, Elise, Howell, Steve B., Bieryla, Allyson, Heng, Kevin, Knutson, Heather A., Collins, Karen A., McLeod, Kim K., Berlind, Perry, Brown, Peyton, Calkins, Michael L., de Leon, Jerome P., Esparza-Borges, Emma, Esquerdo, Gilbert A., Fukui, Akihiko, Gan, Tianjun, Girardin, Eric, Gnilka, Crystal L., Ikoma, Masahiro, Jensen, Eric L. N., Kielkopf, John, Kodama, Takanori, Kurita, Seiya, Lester, Kathryn V., Lewin, Pablo, Marino, Giuseppe, Murgas, Felipe, Narita, Norio, Pallé, Enric, Schwarz, Richard P., Stassun, Keivan G., Tamura, Motohide, Watanabe, Noriharu, Benneke, Björn, Ricker, George R., Latham, David W., Vanderspek, Roland, Seager, Sara, Winn, Joshua N., Jenkins, Jon M., Caldwell, Douglas A., Fong, William, Huang, Chelsea X., Mireles, Ismael, Schlieder, Joshua E., Shiao, Bernie, Villaseñor, Jesus Noel
Publikováno v:
AJ, 162, 256 (2021)
We report the discovery of an ultrahot Jupiter with an extremely short orbital period of $0.67247414\,\pm\,0.00000028$ days ($\sim$16 hr). The $1.347 \pm 0.047$ $R_{\rm Jup}$ planet, initially identified by the Transiting Exoplanet Survey Satellite (
Externí odkaz:
http://arxiv.org/abs/2111.12074
Autor:
Fausnaugh, Michael, Morgan, Ed, Vanderspek, Roland, Pepper, Joshua, Burke, Christopher J., Levine, Alan M., Rudat, Alexander, Villaseñor, Jesus Noel S., Vezie, Michael, Goeke, Robert F., Ricker, George R., Latham, David W., Seager, S., Winn, Joshua N., Jenkins, Jon M., Bakos, G. A., Barclay, Thomas, Berta-thompson, Zachory K., Bouma, Luke G., Boyd, Patricia T., Brasseur, C. E., Burt, Jennifer, Caldwell, Douglas A., Charbonneau, David, Christensen-dalsgaard, J., Clampin, Mark, Collins, Karen A., Colón, Knicole D., De Lee, Nathan, Dunham, Edward, Fleming, Scott W., Fong, William, Soto, Aylin Garcia, Gaudi, B. Scott, Guerrero, Natalia M., Hesse, Katharine, Holman, Matthew J., Huang, Chelsea X., Kaltenegger, Lisa, Lissauer, Jack J., Mcdermott, Scott, Mclean, Brian, Mireles, Ismael, Mullally, Susan E., Oelkers, Ryan J., Paegert, Martin, Pal, Andras, Quintana, Elisa V., Rinehart, S. A., Rodriguez, David R., Rose, Mark, Sasselov, Dimitar D., Schlieder, Joshua E., Sha, Lizhou, Shporer, Avi, Smith, Jeffrey C., Stassun, Keivan G., Tenenbaum, Peter, Ting, Eric B., Torres, Guillermo, Twicken, Joseph D., Vanderburg, Andrew, Wohler, Bill, Yu, Liang
We describe the target selection procedure by which stars are selected for 2-minute and 20-second observations by TESS. We first list the technical requirements of the TESS instrument and ground systems processing that limit the total number of targe
Externí odkaz:
http://arxiv.org/abs/2109.02665
Autor:
Osborn, Ares, Armstrong, David J., Cale, Bryson, Brahm, Rafael, Wittenmyer, Robert A., Dai, Fei, Crossfield, Ian J. M., Bryant, Edward M., Adibekyan, Vardan, Cloutier, Ryan, Collins, Karen A., Mena, E. Delgado, Fridlund, Malcolm, Hellier, Coel, Howell, Steve B., King, George W., Lillo-Box, Jorge, Otegi, Jon, Sousa, S., Stassun, Keivan G., Matthews, Elisabeth C., Ziegler, Carl, Ricker, George, Vanderspek, Roland, Latham, David W., Seager, S., Winn, Joshua N., Jenkins, Jon M., Acton, Jack S., Addison, Brett C., Anderson, David R., Ballard, Sarah, Barrado, David, Barros, Susana C. C., Batalha, Natalie, Bayliss, Daniel, Barclay, Thomas, Benneke, Björn, Berberian Jr., John, Bouchy, Francois, Bowler, Brendan P., Briceño, César, Burke, Christopher J., Burleigh, Matthew R., Casewell, Sarah L., Ciardi, David, Collins, Kevin I., Cooke, Benjamin F., Demangeon, Olivier D. S., Díaz, Rodrigo F., Dorn, C., Dragomir, Diana, Dressing, Courtney, Dumusque, Xavier, Espinoza, Néstor, Figueira, P., Fulton, Benjamin, Furlan, E., Gaidos, E., Geneser, C., Gill, Samuel, Goad, Michael R., Gonzales, Erica J., Gorjian, Varoujan, Günther, Maximilian N., Helled, Ravit, Henderson, Beth A., Henning, Thomas, Hogan, Aleisha, Hojjatpanah, Saeed, Horner, Jonathan, Howard, Andrew W., Hoyer, Sergio, Huber, Dan, Isaacson, Howard, Jenkins, James S., Jensen, Eric L. N., Jordán, Andrés, Kane, Stephen R., Kidwell Jr., Richard C., Kielkopf, John, Law, Nicholas, Lendl, Monika, Lund, M., Matson, Rachel A., Mann, Andrew W., McCormac, James, Mengel, Matthew W., Morales, Farisa Y., Nielsen, Louise D., Okumura, Jack, Osborn, Hugh P., Petigura, Erik A., Plavchan, Peter, Pollacco, Don, Quintana, Elisa V., Raynard, Liam, Robertson, Paul, Rose, Mark E., Roy, Arpita, Reefe, Michael, Santerne, Alexandre, Santos, Nuno C., Sarkis, Paula, Schlieder, J., Schwarz, Richard P., Scott, Nicholas J., Shporer, Avi, Smith, A. M. S., Stibbard, C., Stockdale, Chris, Strøm, Paul A., Twicken, Joseph D., Tan, Thiam-Guan, Tanner, A., Teske, J., Tilbrook, Rosanna H., Tinney, C. G., Udry, Stephane, Villaseñor, Jesus Noel, Vines, Jose I., Wang, Sharon X., Weiss, Lauren M., West, Richard G., Wheatley, Peter J., Wright, Duncan J., Zhang, Hui, Zohrabi, F.
We present the bright (V$_{mag} = 9.12$), multi-planet system TOI-431, characterised with photometry and radial velocities. We estimate the stellar rotation period to be $30.5 \pm 0.7$ days using archival photometry and radial velocities. TOI-431b is
Externí odkaz:
http://arxiv.org/abs/2108.02310
Autor:
Ikwut-Ukwa, Mma, Rodriguez, Joseph E., Quinn, Samuel N., Zhou, George, Vanderburg, Andrew, Ali, Asma, Bunten, Katya, Gaudi, B. Scott, Latham, David W., Howell, Steve B., Huang, Chelsea X., Bieryla, Allyson, Collins, Karen A., Carmichael, Theron W., Rabus, Markus, Eastman, Jason D., Collins, Kevin I., Tan, Thiam-Guan, Schwarz, Richard P., Myers, Gordon, Stockdale, Chris, Kielkopf, John F., Radford, Don J., Oelkers, Ryan J., Jenkins, Jon M., Ricker, George R., Seager, Sara, Vanderspek, Roland K., Winn, Joshua N., Burt, Jennifer, Butler, R. Paul, Calkins, Michael L., Crane, Jeffrey D., Gnilka, Crystal L., Esquerdo, Gilbert A., Fong, Wlliam, Kreidberg, Laura, Mink, Jessica, Rodriguez, David R., Schlieder, Joshua E., Schectman, Stephen, Shporer, Avi, Teske, Johanna, Ting, Eric B., Villasenor, Jesus Noel, Yahalomi, Daniel A.
We report the discovery of two short-period massive giant planets from NASA's Transiting Exoplanet Survey Satellite (TESS). Both systems, TOI-558 (TIC 207110080) and TOI-559 (TIC 209459275), were identified from the 30-minute cadence Full Frame Image
Externí odkaz:
http://arxiv.org/abs/2102.02222
Autor:
Schlecker, Martin, Kossakowski, Diana, Brahm, Rafael, Espinoza, Néstor, Henning, Thomas, Carone, Ludmila, Molaverdikhani, Karan, Trifonov, Trifon, Mollière, Paul, Hobson, Melissa J., Jordán, Andrés, Rojas, Felipe I., Klahr, Hubert, Sarkis, Paula, Bakos, Gáspár Á., Bhatti, Waqas, Osip, David, Suc, Vincent, Ricker, George, Vanderspek, Roland, Latham, David W., Seager, Sara, Winn, Joshua N., Jenkins, Jon M., Vezie, Michael, Villaseñor, Jesus Noel, Rose, Mark E., Rodriguez, David R., Rodriguez, Joseph E., Quinn, Samuel N., Shporer, Avi
The orbital parameters of warm Jupiters serve as a record of their formation history, providing constraints on formation scenarios for giant planets on close and intermediate orbits. Here, we report the discovery of TIC 237913194b, detected in full f
Externí odkaz:
http://arxiv.org/abs/2010.03570
Autor:
Jenkins, James S., Díaz, Matías R., Kurtovic, Nicolás T., Espinoza, Néstor, Vines, Jose I., Rojas, Pablo A. Peña, Brahm, Rafael, Torres, Pascal, Cortés-Zuleta, Pía, Soto, Maritza G., Lopez, Eric D., King, George W., Wheatley, Peter J., Winn, Joshua N., Ciardi, David R., Ricker, George, Vanderspek, Roland, Latham, David W., Seager, Sara, Jenkins, Jon M., Beichman, Charles A., Bieryla, Allyson, Burke, Christopher J., Christiansen, Jessie L., Henze, Christopher E., Klaus, Todd C., McCauliff, Sean, Mori, Mayuko, Narita, Norio, Nishiumi, Taku, Tamura, Motohide, de Leon, Jerome Pitogo, Quinn, Samuel N., Villaseñor, Jesus Noel, Vezie, Michael, Lissauer, Jack J., Collins, Karen A., Collins, Kevin I., Isopi, Giovanni, Mallia, Franco, Ercolino, Andrea, Petrovich, Cristobal, Jordán, Andrés, Acton, Jack S., Armstrong, David J., Bayliss, Daniel, Bouchy, François, Belardi, Claudia, Bryant, Edward M., Burleigh, Matthew R., Cabrera, Juan, Casewell, Sarah L., Chaushev, Alexander, Cooke, Benjamin F., Eigmüller, Philipp, Erikson, Anders, Foxell, Emma, Gänsicke, Boris T., Gill, Samuel, Gillen, Edward, Günther, Maximilian N., Goad, Michael R., Hooton, Matthew J., Jackman, James A. G., Louden, Tom, McCormac, James, Moyano, Maximiliano, Nielsen, Louise D., Pollacco, Don, Queloz, Didier, Rauer, Heike, Raynard, Liam, Smith, Alexis M. S., Tilbrook, Rosanna H., Titz-Weider, Ruth, Turner, Oliver, Udry, Stéphane, Walker, Simon. R., Watson, Christopher A., West, Richard G., Palle, Enric, Ziegler, Carl, Law, Nicholas, Mann, Andrew W.
About one out of 200 Sun-like stars has a planet with an orbital period shorter than one day: an ultra-short-period planet (Sanchis-ojeda et al. 2014; Winn et al. 2018). All of the previously known ultra-short-period planets are either hot Jupiters,
Externí odkaz:
http://arxiv.org/abs/2009.12832